Imaging the Cosmic Microwave Background with the Arcminute Cosmology Bolometer Array Receiver

Details Imaging the Cosmic Microwave Background with the Arcminute Cosmology Bolometer Array Receiver Imaging the Cosmic Microwave Background with the Arcminute Cosmology Bolometer Array Receiver

Jan 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005iaus..216...43p&link_type=abstract

Maps of the Cosmos, Proceedings of IAU Symposium No. 216, held during the IAU General Assembly XXV in Sydney, Australia, 14-17 J

Mathematics

Logic

Scientific paper

Arcminute Cosmology Bolometer Array Receiver (Acbar) is a multifrequency millimeter-wave receiver optimized for observations of the Cosmic Microwave Background (CMB) and the Sunyaev-Zel'dovich (SZ) effect in clusters of galaxies. Acbar was installed on the 2.1 m Viper telescope at the South Pole in January 2001 and the results presented here incorporate data through July 2002. The power spectrum of the CMB at 150 GHz over the range ℓ=150 - 3000 measured by Acbar is presented along with estimates for the values of the cosmological parameters within the context of ΛCDM models. The inclusion of Ω_Λ greatly improves the fit to the power spectrum. Three-frequency images of the SZ decrement/increment are also presented for the galaxy cluster 1E0657-67.

Affiliated with

Also associated with

No associations

Rating

Imaging the Cosmic Microwave Background with the Arcminute Cosmology Bolometer Array Receiver does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Imaging the Cosmic Microwave Background with the Arcminute Cosmology Bolometer Array Receiver, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Imaging the Cosmic Microwave Background with the Arcminute Cosmology Bolometer Array Receiver will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-808047